Optical counterparts of the nearest ultraluminous X-ray sources
Jeanette C. Gladstone (1), Chris Copperwheat (2), Craig O. Heinke (1),, Timothy P. Roberts (3), Taylor F. Cartwright (1,4), Andrew J. Levan (5), Mike, R. Goad (6). ((1) University of Alberta, (2) Liverpool John Moores, University, (3) University of Durham

TL;DR
This study surveys optical counterparts of nearby ultraluminous X-ray sources using Hubble data, identifying potential companion stars and constraining their types and properties to better understand ULX systems.
Contribution
It provides the first comprehensive optical counterpart analysis of ULXs within 5 Mpc, including candidate spectral types and constraints on donor star and black hole properties.
Findings
13 +/- 5 ULXs have true optical counterparts.
O-type companions are ruled out in 20 cases.
Constraints on black hole masses are established for 7 ULXs.
Abstract
We present a photometric survey of the optical counterparts of ultraluminous X-ray sources (ULXs) observed with the Hubble Space Telescope in nearby (< 5 Mpc) galaxies. Of the 33 ULXs with Hubble & Chandra data, 9 have no visible counterpart, placing limits on their M_V of ~ -4 to -9, enabling us to rule out O-type companions in 4 cases. The refined positions of two ULXs place them in the nucleus of their host galaxy. They are removed from our sample. Of the 22 remaining ULXs, 13 have one possible optical counterpart, while multiple are visible within the error regions of other ULXs. By calculating the number of chance coincidences, we estimate that 13 +/- 5 are the true counterparts. We attempt to constrain the nature of the companions by fitting the SED and M_V to obtain candidate spectral types. We can rule out O-type companions in 20 cases, while we find that one ULX (NGC 253 ULX2)…
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